Discovery of the binary nature of the magnetospheric B-type star $\rho$ Oph A

TL;DR

This study reveals that the B-type star $ ho$ Oph A is a binary system with the magnetic field associated with the smaller component, exhibiting a strong, nearly dipolar magnetosphere with observable eclipses and asymmetries.

Contribution

It is the first to identify $ ho$ Oph A as a binary with a magnetic component, measuring a stronger magnetic field and modeling its magnetosphere with detailed spectropolarimetric data.

Findings

$ ho$ Oph A is a spectroscopic binary with magnetic field in the smaller star.

The magnetic field of the smaller star is approximately 4 kG, twice as strong as previously reported.

The magnetosphere shows prominent asymmetries and magnetospheric eclipses similar to $\sigma$ Ori E.

Abstract

The nearby B-type star $\rho$ Oph A was recently identified as a rapidly rotating magnetic B-type star with variable radio and X-ray emission consistent with a magnetospheric origin. We present a high-resolution spectropolarimetric time series obtained with ESPaDOnS, which we use to perform a magnetic analysis using least-squares deconvolution (LSD). We find that $\rho$ Oph A is a spectroscopic binary consisting of two B-type stars with masses of about 8 and 10 $M_\odot$ on a slightly eccentric 88-day orbit, with the magnetic field being associated with the smaller Ab component. This leads to $\rho$ Oph Ab's 4 kG surface magnetic dipole being approximately twice as strong as the previously reported 2 kG. The oblique rotator model derived from the longitudinal magnetic field curve agrees well with the LSD Stokes $V$ profiles, indicating that the magnetic field is likely to be very nearly dipolar. The orbital and rotational axes appear to be aligned. We report for the first time $\rho$ Oph Ab's magnetospheric H$\alpha$ emission, which is consistent with an origin in a centrifugal magnetosphere. We also demonstrate that $\rho$ Oph Ab's light curve can be recovered from the previously reported {\em Kepler-2} light curve of $\rho$ Oph C, and that it demonstrates prominent magnetospheric eclipses similar to those of $\sigma$ Ori E, and which can be reproduced using a dipolar Rigidly Rotating Magnetosphere model. Both H$\alpha$ and the light curve are indicative of a strongly asymmetric magnetosphere. All indications are that $\rho$ Oph Ab's magnetic field is essentially dipolar, meaning that contributions from higher-order multipoles probably cannot explain the strong asymmetry in the magnetosphere. Only two other stars show comparable degrees of asymmetry, both of which are also close binaries, suggesting that binarity can affect the magnetospheric plasma distributions.